High energy emission from starburst galaxies
Abstract
The star formation (SF) can be regarded as an engine powering the light emission of spiral galaxies at several wavelengths. SF activity also plays a significant role in the evolution of galaxies. In this thesis we focus on the X-ray emission from processes related to star formation. Several kinds of sources concur to X-ray emission, X-ray binaries and hot plasma being the most important. We begin with a review of the infrared, radio and X-ray emission from star forming galaxies. In the second chapter we explore the quantitative relationships between the total X-ray, radio and infrared luminosities for a sample of 23 star forming galaxies. It is found that linear correlations hold between the luminosities in the above bands. In the third chapter we show, by analyzing a sample of 11 high redshift galaxies in the Hubble Deep Field, that the linear correlations may be extended up to z~1. In the fourth chapter we turn to an analysis of the luminosity function and number counts of star forming galaxies; we show that the number density of normal galaxies at faint X-ray fluxes (10^-17 -- 10^-15 erg/s/cm2) is very well defined. The fifth chapter offers a first insight into a different aspect of galaxy evolution, i.e. whether is it possible to determine the metallicity enhancements in a starburst episode. An interesting, yet problematic, picture of metal enrichment of the interstellar matter arises from an analysis of the X-ray and near infrared spectra of M82. Finally, a summary is offered of the work here described.
Cite
@article{arxiv.astro-ph/0407140,
title = {High energy emission from starburst galaxies},
author = {Piero Ranalli},
journal= {arXiv preprint arXiv:astro-ph/0407140},
year = {2009}
}
Comments
PhD thesis. 114 pages with many figures and 7 colour plates. Some figures have been degraded to match size limits. Version with full-resolution figures is at http://urania.bo.astro.it/dottorandi/pranalli-phdthesis.pdf